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相关论文: Fine-Tuning Solution for Hybrid Inflation in Dissi…

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We introduce a new class of models of chaotic inflation inspired by the superconformal approach to supergravity. This class of models allows a functional freedom of choice of the inflaton potential V = |f(\phi)|^2. The simplest model of…

高能物理 - 理论 · 物理学 2010-11-22 Renata Kallosh , Andrei Linde

Quantum and thermal fluctuations of an irrotational fluid are studied across the transition regime connecting a protoinflationary phase of decelerated expansion to an accelerated epoch driven by a single inflaton field. The…

高能物理 - 理论 · 物理学 2015-06-04 Massimo Giovannini

We clarify inflaton models by considering them as effective field theories in the Ginzburg-Landau spirit.In this new approach, the precise form of the inflationary potential is constructed from the present WMAP data, and a useful scheme is…

天体物理学 · 物理学 2009-11-10 D. Cirigliano , H. J. de Vega , N. G. Sanchez

We explore how disorder and interactions conspire in lattice models with sequentially activated hopping to produce novel k-body (or many-body) localized phases. Specifically, we show that when disorder is added to the set of interacting…

统计力学 · 物理学 2022-12-20 Matthew Wampler , Israel Klich

We study the phenomenon of discrete symmetry breaking during the inflationary epoch, using a model-independent approach based on the effective field theory of inflation. We work in a context where both time reparameterization symmetry and…

高能物理 - 理论 · 物理学 2015-08-19 Dario Cannone , Jinn-Ouk Gong , Gianmassimo Tasinato

Inflation generally assumes a field with nonzero potential that leads to inflationary expansion happening at arbitrarily early times. We demonstrate potentially observable consequences of inflation with a finite initial time in a model in…

高能物理 - 理论 · 物理学 2025-12-05 Rashmish K. Mishra , Michael Nee , Lisa Randall

We consider the non-supersymmetric models of chaotic (driven by a quadratic potential) and hybrid inflation, taking into account the minimal possible radiative corrections to the inflationary potential. We show that two simple coupling…

宇宙学与河外天体物理 · 物理学 2015-03-13 C. Pallis

In this thesis we will primarily demonstrate how additional scalar degrees of freedom - which are motivated from many high-energy embeddings - open up new observational windows onto the physics of inflation. We construct a Bayesian…

宇宙学与河外天体物理 · 物理学 2019-06-11 Robert J. Hardwick

Stochastic effects in generic scenarios of inflation with multiple fields are investigated. First passage time techniques are employed to calculate the statistical moments of the number of inflationary $e$-folds, which give rise to all…

宇宙学与河外天体物理 · 物理学 2017-01-25 Vincent Vennin , Hooshyar Assadullahi , Hassan Firouzjahi , Mahdiyar Noorbala , David Wands

We study and analyze the dynamic properties of both canonical and noncanonical warm inflationary models with dissipative effects. We consider different models of canonical warm inflation with different dissipative coefficients and prove…

广义相对论与量子宇宙学 · 物理学 2018-08-24 Xi-Bin Li , Yang-Yang Wang , He Wang , Jian-Yang Zhu

We consider a variant of Hybrid Inflation, where inflation is driven by two interacting scalar fields, one of which has a `Mexican hat' potential and the other a quartic potential. Given the appropriate initial conditions one of the fields…

天体物理学 · 物理学 2016-08-24 David Roberts , Andrew R Liddle , David H Lyth

The effective equation of motion is derived for a scalar field interacting with other fields in a Friedman-Robertson-Walker background space-time. The dissipative behavior reflected in this effective evolution equation is studied both in…

高能物理 - 唯象学 · 物理学 2008-11-26 Arjun Berera , Rudnei O. Ramos

How sensitive are the predictions of inflation to pre-inflationary conditions when the number of efolds of inflation is not too large? In an attempt to address this question, we consider a simple model where the inflationary era is preceded…

高能物理 - 理论 · 物理学 2016-01-27 Sina Bahrami , Eanna E. Flanagan

The evolution of a scalar field is explored taking into account the presence of a background fluid in a positively curved Universe in the framework of loop quantum cosmology. Though the mechanism that provides the initial conditions for…

天体物理学 · 物理学 2009-11-13 N. J. Nunes

In an alternative mechanism recently proposed, adiabatic cosmological perturbations are generated at the decay of the inflaton field due to small fluctuations of its coupling to matter. This happens whenever the coupling is governed by the…

天体物理学 · 物理学 2009-11-10 Rouzbeh Allahverdi

Inflation models can have an early phase of inflation where the evolution of the inflaton is driven by quantum fluctuations before entering the phase driven by the slope of the scalar field potential. For a Coleman-Weinberg potential this…

宇宙学与河外天体物理 · 物理学 2013-03-06 Arjun Berera , Raghavan Rangarajan

We analyze constraints on parameters characterizing the pre-inflating universe in an open inflation model with a present slightly open $\Lambda$CDM universe. We employ an analytic model to show that for a broad class of inflation-generating…

宇宙学与河外天体物理 · 物理学 2015-12-17 G. J. Mathews , I. -S. Suh , N. Q. Lan , T. Kajino

We show that the standard model Higgs field can realize the quadratic chaotic inflation, if the kinetic term is significantly modified at large field values. This is a simple realization of the so-called running kinetic inflation. The point…

高能物理 - 唯象学 · 物理学 2014-06-05 Kazunori Nakayama , Fuminobu Takahashi

Stochastic effects in multi-field inflationary scenarios are investigated. A hierarchy of diffusion equations is derived, the solutions of which yield moments of the numbers of inflationary $e$-folds. Solving the resulting partial…

高能物理 - 理论 · 物理学 2016-08-24 Hooshyar Assadullahi , Hassan Firouzjahi , Mahdiyar Noorbala , Vincent Vennin , David Wands

In this brief review we introduce the methods of quantum field theory out of equilibrium and study the non-equilibrium aspects of phase transitions. Specifically we critically study the picture of the ``slow-roll'' phase transition in the…

高能物理 - 理论 · 物理学 2009-09-25 D. Boyanovsky , H. J. de Vega , R. Holman